Zobrazeno 1 - 10
of 892
pro vyhledávání: '"A. Sanchez-Lavega"'
Autor:
Harkett, Jake, Fletcher, Leigh N., King, Oliver R. T., Roman, Michael T., Melin, Henrik, Hammel, Heidi B., Hueso, Ricardo, Sánchez-Lavega, Agustín, Wong, Michael H., Milam, Stefanie N., Orton, Glenn S., de Kleer, Katherine, Irwin, Patrick G. J., de Pater, Imke, Fouchet, Thierry, Rodríguez-Ovalle, Pablo, Fry, Patrick M., Showalter, Mark R.
Publikováno v:
JGR:Planets, 129, e2024JE008415
Jupiter's Great Red Spot (GRS) was mapped by the James Webb Space Telescope (JWST)/Mid-Infrared Instrument (4.9-27.9 micron) in July and August 2022. These observations took place alongside a suite of visual and infrared observations from; Hubble, JW
Externí odkaz:
http://arxiv.org/abs/2410.02468
Autor:
M. T. Lemmon, M. D. Smith, D. Viudez‐Moreiras, M. de laTorre‐Juarez, A. Vicente‐Retortillo, A. Munguira, A. Sanchez‐Lavega, R. Hueso, G. Martinez, B. Chide, R. Sullivan, D. Toledo, L. Tamppari, T. Bertrand, J. F. Bell III, C. Newman, M. Baker, D. Banfield, J. A. Rodriguez‐Manfredi, J. N. Maki, V. Apestigue
Publikováno v:
Geophysical Research Letters, Vol 49, Iss 17, Pp n/a-n/a (2022)
Abstract Rovers and landers on Mars have experienced local, regional, and planetary‐scale dust storms. However, in situ documentation of active lifting within storms has remained elusive. Over 5–11 January 2022 (LS 153°–156°), a dust storm pa
Externí odkaz:
https://doaj.org/article/4a0559d66076471b8e1f16369fe796d4
Autor:
Sánchez-Lavega, Agustín, García-Melendo, Enrique, Legarreta, Jon, Miró, Arnau, Soria, Manel, Ahrens-Velásquez, Kevin
Publikováno v:
Geophysical Research Letters, Volume 51, Issue 12, 28 June 2024, e2024GL108993
Jupiter's Grat Red Spot (GRS) is the largest and longest-lived vortex of all solar system planets but its lifetime is debated and its formation mechanism remains hidden. G. D. Cassini discovered in 1665 the presence of a dark oval at the GRS latitude
Externí odkaz:
http://arxiv.org/abs/2406.13222
Autor:
Rodríguez-Ovalle, Pablo, Fouchet, Thierry, Guerlet, Sandrine, Cavalié, Thibault, Hue, Vincent, López-Puertas, Manuel, Lellouch, Emmanuel, Sinclair, James A., de Pater, Imke, Fletcher, Leigh N., Wong, Michael H., Harkett, Jake, Orton, Glenn S., Hueso, Ricardo, Sánchez-Lavega, Agustín, Stallard, Tom S., Bockelee-Morvan, Dominique, King, Oliver, Roman, Michael T., Melin, Henrik
Jupiters south polar region was observed by JWST Mid Infrared Instrument in December 2022. We used the Medium Resolution Spectrometer mode to provide new information about Jupiters South Polar stratosphere. The southern auroral region was visible and
Externí odkaz:
http://arxiv.org/abs/2406.08133
Autor:
Liming Li, X. Jiang, R. A. West, P. J. Gierasch, S. Perez-Hoyos, A. Sanchez-Lavega, L. N. Fletcher, J. J. Fortney, B. Knowles, C. C. Porco, K. H. Baines, P. M. Fry, A. Mallama, R. K. Achterberg, A. A. Simon, C. A. Nixon, G. S. Orton, U. A. Dyudina, S. P. Ewald, R. W. Schmude
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-10 (2018)
Radiant energy budgets and internal heat play a key role in the evolution of planets. Here, the authors analyze data from the Cassini mission to show that Jupiter’s radiant energy and internal heat budgets are significantly larger than previous est
Externí odkaz:
https://doaj.org/article/92b1ada5213949ffbad5921127c4243c
Publikováno v:
J. Geophys. Res. Planets (2015) 120 155-176
We analyze data retrieved by the Imaging Science System onboard the Cassini spacecraft to study the horizontal velocity and vorticity fields of Saturn's Polar Regions (latitudes 60-90$^\circ$N in June-December 2013 and 60-90$^\circ$S in October 2006
Externí odkaz:
http://arxiv.org/abs/2402.07468
Autor:
Sánchez-Lavega, A., del Río-Gaztelurrutia, T., Hueso, R., Pérez-Hoyos, S., García-Melendo, E., Antuñano, A., Mendikoa, I., Rojas, J. F., Lillo, J., Barrado-Navascués, D., Gomez-Forrellad, J. M., Go, C., Peach, D., Barry, T., Milika, D. P., Nicholas, P., Wesley, A., Team, the IOPW-PVOL
Publikováno v:
Geophys. Res. Lett. (2014) 41 1425-1431
We investigate the long-term motion of Saturn's North-Pole Hexagon and the structure of its associated eastward jet, using Cassini ISS and ground-based images from 2008 to 2014. We show that both are persistent features that have survived the long po
Externí odkaz:
http://arxiv.org/abs/2402.06371
Publikováno v:
Planetary and Space Science, vol. 81, 65-73 (2013)
Thermal radiation becomes a prominent feature in the continuum spectrum of Venus longwards of $\sim$3 $\mu$m. The emission is traceable to the upper cloud and haze layers in the planet's mesosphere. Venus' thermal radiation spectrum is punctuated by
Externí odkaz:
http://arxiv.org/abs/2402.03926
Publikováno v:
Journal of Geophysical Research: Planets, vol. 121, 574-593 (2016)
Venus' atmosphere shows highly variable warm vortices over both of the planet's poles. The nature of the mechanism behind their formation and properties is still unknown. Potential vorticity is a conserved quantity when advective processes dominate o
Externí odkaz:
http://arxiv.org/abs/2402.00679
Publikováno v:
Icarus, vol. 245, 16-31 (2015)
The Venus thermal radiation spectrum exhibits the signature of $CO_2$ absorption bands. By means of inversion techniques, those bands enable the retrieval of atmospheric temperature profiles. We have analyzed VIRTIS-M-IR night-side data obtaining hig
Externí odkaz:
http://arxiv.org/abs/2401.17946